WD-2332+2347 is a white dwarf star with no planets orbiting it.
|Age||6 Billion Years|
|Type||White Dwarf Star|
|Number Of Planets||0|
|Mass||1.3× that of the Sun|
|Surface Temperature||14,432 F|
|Core Temperature||198,000 F|
|Distance From Centre Of Galaxy||3,000 Light Years|
|Orbital Period||34,453,443 Years|
|Surface Gravity||333,000× that of Earth|
About 6 billion years ago a nebulae formed that formed just a white giant star about 1.3 times the mass of the Sun, however being so massive it started using up it's energy more rapidly than a low mass star or a lower mass medium star would and about 3 billion years ago it started to run out of hydrogen and it's core heated up tremendously as the star started to contract and when the star's core reached 180,000,000 F it started to fuse Helium into Carbon and Oxygen and started to balloon out into a Red Giant, but once again the initial mass of the star caused this to be short lived as well, about 8 million years later it ran out of helium and started to puff out it's outer layers into a planetary nebula and it's cored started to contract under gravity until Electron Degeneracy Pressure kicked in and it stopped contracting with a diameter of 14,326 km, it slowly cooled off from a surface temperature of 16,000 F to about 14,432 F where it is at today.
- In about 110 billion years it'll have lost enough of it's radiant energy from it's lifetime of energy from when it was a Main Sequence Star to a cold dead black dwarf star and it'll stop shining altogether, and it's surface temperature will be just 2K, a couple degrees above absolute zero.